To find the ratio of the transition energy for the $2p \rightarrow 1s$ transition in \(He^+\) to that in the H atom, we need to consider the Rydberg formula for calculating the energy of the \( nth \) level in hydrogen-like atoms. The formula for the energy levels is given by:
\(E_n = -Z^2 \frac{R_H}{n^2}\)
where:
For a transition from the \(2p\) level (\(n=2\)) to the \(1s\) level (\(n=1\)), the energy change is given by:
\(\Delta E = E_1 - E_2 = -Z^2 \frac{R_H}{1^2} + Z^2 \frac{R_H}{2^2}\)
Simplifying this expression gives:
\(\Delta E = -Z^2 R_H + \frac{Z^2 R_H}{4} = -\frac{3Z^2 R_H}{4}\)
Now, let's calculate the transition energy ratio between \(He^+\) and \(H\):
The ratio of the transition energies is:
\(\text{Ratio} = \frac{\Delta E_{He^+}}{\Delta E_{H}} = \frac{-3R_H}{-\frac{3R_H}{4}} = 4\)
Therefore, the correct answer is 4. This shows that the energy of the \(2p \rightarrow 1s\) transition in \(He^+\) is four times that in the hydrogen atom.
The figures below show:
Which of the following points in Figure 2 most accurately represents the nodal surface shown in Figure 1?
The wavelength of spectral line obtained in the spectrum of Li$^{2+}$ ion, when the transition takes place between two levels whose sum is 4 and difference is 2, is